\begin{table}%t1
\caption{\label{T1}Models parameters. }
%\centerline
 {\small \begin{tabular}{ccccccc}
\noalign{\smallskip}
\hline \hline \noalign{\smallskip}
Model~& Threshold & $\nu$ (4--6--8--10--12--14~kpc) & $\tau$ & $\Sigma_{\rm halo}$ & Infall law & SFR \\
\noalign{\smallskip} \hline \noalign{\smallskip}
C08 & yes & const & / & / & cosmological & Eq.~(1) \\
C97 & yes & const & 1.03 $\cdot$ $R$ - 1.27 & const & two-infall law & Eq.~(1) \\
1 & no & const & / & / & cosmological & Eq.~(1) \\
2 & no & 8.0--4.0--1.0--0.5--0.2--0.05 & / & / & cosmological & Eq.~(1) \\
3 & no & 4.0--1.0--0.1 & / & / & cosmological with inside-out & Eq.~(1) \\
4 & no & const & const & const & two-infall law & Eq.~(1) \\
5 & no & const & 1.03 $\cdot$ $R$--1.27 & const & two-infall law & Eq.~(1) \\
6 & no & 9.0--3.0--1.0--0.3--0.1--0.03 & $1.03 \cdot R$--1.27 & $\propto$ 1/$R$ & two-infall law & Eq.~(1) \\
7 & no & $0.1 \cdot 8/R$ & const & / & one-infall law & Eq.~(2) \\
\noalign{\smallskip}
\hline
\end{tabular}}
\medskip
The second column indicates the presence or absence of a threshold, 
the third column the type of SF efficiency, the fourth whether the galaxy forms inside-out and the fifth  whether the halo density is a constant or a function of radius. In the sixth column, we show the  type of infall law used, and in the seventh column the SFR. The values of $\nu$ for Model~3 are for  2.5, 7.5, and 12.5~kpc.
\end{table}